SUMMARY
The concept of an expanding universe was first proposed by Alexander Friedmann in the early 1920s through his solutions to the Einstein Field Equations (EFE). However, it was Edwin Hubble's observations in 1929 that provided the first definitive evidence supporting this theory, demonstrating the correlation between redshift and distance. While Friedmann's work laid the groundwork, Hubble's empirical data established the expanding universe as a cornerstone of modern cosmology. Einstein initially rejected the idea of an expanding universe, favoring a static model, but ultimately accepted the evidence presented by Hubble.
PREREQUISITES
- Understanding of Einstein Field Equations (EFE)
- Familiarity with redshift and its significance in cosmology
- Knowledge of the historical context of early 20th-century astrophysics
- Awareness of key figures in cosmology, including Hubble and Friedmann
NEXT STEPS
- Research the implications of Hubble's Law in modern cosmology
- Study the Friedmann equations and their role in cosmological models
- Explore the historical development of the Big Bang theory and its challengers
- Investigate the impact of redshift measurements on our understanding of the universe's expansion
USEFUL FOR
Astronomers, astrophysicists, students of cosmology, and anyone interested in the historical development of theories regarding the universe's expansion.